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2Physics

2Physics Quote:
"Many of the molecules found by ROSINA DFMS in the coma of comet 67P are compatible with the idea that comets delivered key molecules for prebiotic chemistry throughout the solar system and in particular to the early Earth increasing drastically the concentration of life-related chemicals by impact on a closed water body. The fact that glycine was most probably formed on dust grains in the presolar stage also makes these molecules somehow universal, which means that what happened in the solar system could probably happen elsewhere in the Universe."
-- Kathrin Altwegg and the ROSINA Team

(Read Full Article: "Glycine, an Amino Acid and Other Prebiotic Molecules in Comet 67P/Churyumov-Gerasimenko"
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Thursday, February 21, 2008

Observation of the Spin Hall Effect of Light

Hosten-KwaitOnur Hosten (left) and Paul Kwiat (right) [Photo credit: L. Brian Stauffer]

Physicists Onur Hosten and Paul G. Kwiat, at the University of Illinois at Urbana-Champaign showed that light exhibits a Spin Hall effect, analogous to the Spin Hall effect in electronic systems, showing the universality of the effect for particles of different nature. The researchers used a novel technique from quantum weak measurements to enhance the tiny Spin Hall displacements prior to observation.

Whenever the propagation direction of a beam of light changes due to a variation in the refractive index of the medium (in the experiment, refraction at an air-glass interface serves this purpose), the beam center experiences a spin-dependent (or circular polarization-dependent) displacement perpendicular both to the initial propagation direction and the change in the propagation direction, i.e. a lateral shift. Two different spin components (parallel and anti-parallel to the propagation direction) acquire opposite displacements. This is the spin Hall effect as it applies to light. Therefore, when a beam of linearly polarized light (which is an equal combination of spin parallel and anti-parallel to the propagation direction) changes direction, the beam slightly splits into two beams, each containing different spin states.

Spin Hall Effect Animation (Click to see)Figure 1: Spin Hall effect of Light. (Click on figure to watch it) In the animation, a beam of linearly polarized light incident on an air-glass interface slightly splits into its two spin components -- spin parallel or anti-parallel to the propagation direction (or right and left circular polarizations) -- upon refraction at the interface. [Animation credit: Onur Hosten]

The effect takes place due to conservation of angular momentum (spin plus orbital). Due to the rotational symmetry around the axis perpendicular to the interface (z-axis), the total angular momentum of light around this axis has to be conserved. Assume that, initially the spin angular momentum of light is either parallel or anti-parallel to the propagation direction, and has a certain component along the z-axis. When light refracts at the interface, the spin still remains either parallel or anti-parallel to the new propagation direction. But this time the spin makes a different angle with the z-axis, therefore the spin angular momentum component along the z-axis changes. The spin Hall effect compensates for this change in the angular momentum component, and light acquires an orbital angular momentum by shifting itself laterally from the z-axis.

In the experiment a linearly polarized laser beam was incident on a glass prism at an angle. Upon refraction, the two different spin components acquired opposite displacements out of the plane of incidence. Because the separation between these two beams was only on the order of nanometers, and the beam widths themselves on the order of millimeters, the two beams overlap to a great extent. The researchers measured the separation between the two beams using a novel metrological method (quantum weak measurements in pre- and post-selected systems) to measure the miniscule effect.

Essentially, the spin Hall effect performs a weak measurement of the spin state of the photons. If the measurement were to be strong, the beams corresponding to different spin states would completely separate from each other, and one would be able to tell the spin state by looking at the beam position. But, in the University of Illinois experiment, the spin state measurement was a weak measurement, because the beams were still overlapping to a great extent and one could tell only very little about the spin state by looking at the position of the beam.

When the researchers made a particular pre- and post-selection on the polarization state of the photons before and after the weak measurement (i.e., the spin Hall effect), due to an interference effect between the two beams, there resulted an enhancement of the original displacement by a factor of ten thousand. This pre- and post-selection step experimentally amounts to sending the photons through two calcite polarizers, one before and one after the spin Hall effect, oriented at angles almost perpendicular to each other. Therefore, for instance, an angstrom displacement was enhanced to a micron displacement. Then the enhanced displacement was read by a position-sensitive photodiode (a photodiode split into two halves – the difference signal is proportional to the beam displacement). The researchers were thus able to characterize the Spin Hall effect of light with angstrom resolution.

The measurement technique holds further promise for achieving better resolutions. In particular, the researchers believe that by incorporating standard signal modulation and lock-in detection techniques, a resolution of picometers can be achieved. Moreover, the technique is not limited to position measurements; similar tricks in the appropriate experimental conditions will enhance any kind of signal, e.g., position or momentum of any particle, intensity (e.g. photon number) or amplitude (e.g. electric field) of a field.

The researchers think that it would be interesting to demonstrate the case when the index of refraction varies continuously (as opposed to observing the effect at a discrete air-glass interface), which is the analogous case for the spin Hall effect in semiconductors. The researchers are also theoretically looking for systems where they can separate the spin states into two completely separate beams, and use this for both quantum and classical optical information processing applications.

Reference:
"Observation of the Spin Hall Effect of Light via Weak Measurements"
O. Hosten and P. Kwiat,
Science 319, 787 (2008); published online 10 January 2008 (10.1126/Science.1152697).
Link to Abstract
Link to Full text in the website of Kwiat Quantum Information Group

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Thursday, February 14, 2008

Distortions in Large Scale Structures of Galaxies Shed New Light On Dark Energy

Large Scale Structures of galaxies [Image courtesy: European Organisation for Astronomical Research in the Southern Hemisphere (ESO)]

An international team of 51 scientists from 24 institutions took the challenge of performing the measurement of the distribution and motions of thousands of galaxies in the distant Universe using ESO's Very Large Telescope in order to better understand what drives the acceleration of the cosmic expansion. In a recent paper in 'Nature', they report their results which shed new light on the mysterious dark energy that is thought to permeate the Universe.

Ten years ago, astronomers made the stunning discovery that the Universe is expanding at a faster pace today than it did in the past. "Explaining why the expansion of the Universe is currently accelerating is certainly the most fascinating question in modern cosmology," says Luigi Guzzo, lead author of the 'Nature' paper, "We have been able to show that large surveys that measure the positions and velocities of distant galaxies provide us with a new powerful way to solve this mystery."

"The expansion implies that one of two very different possibilities must hold true," explains Enzo Branchini, member of the team, "Either the Universe is filled with a mysterious dark energy which produces a repulsive force that fights the gravitational brake from all the matter present in the Universe, or, our current theory of gravitation is not correct and needs to be modified, for example by adding extra dimensions to space."

Current observations of the expansion rate of the Universe cannot distinguish between these two options. But this international team based their clever technique on a well-known phenomenon, namely the fact that the apparent motion of distant galaxies results from two effects: the global expansion of the Universe that pushes the galaxies away from each other and the gravitational attraction of matter present in the galaxies' neighbourhood that pulls them together, creating the cosmic web of large-scale structures.

"By measuring the apparent velocities of large samples of galaxies over the last thirty years, astronomers have been able to reconstruct a three-dimensional map of the distribution of galaxies over large volumes of the Universe. This map revealed large-scale structures such as clusters of galaxies and filamentary superclusters," says Olivier Le Fèvre, member of the team, "But the measured velocities also contain information about the local motions of galaxies; these introduce small but significant distortions in the reconstructed maps of the Universe. We have shown that measuring this distortion at different epochs of the Universe's history is a way to test the nature of dark energy."

Guzzo and his collaborators have been able to measure this effect by using the VIMOS spectrograph on Melipal, one of the four 8.2-m telescopes that is part of ESO's VLT. As part of the VIMOS-VLT Deep Survey (VVDS), spectra of several thousands of galaxies in a 4-square-degree field (or 20 times the size of the full Moon) at epochs corresponding to about half the current age of the Universe (about 7 billion years ago) were obtained and analysed. This is the largest field ever covered homogeneously by means of spectroscopy to this depth. The team has now collected more than 13,000 spectra in this field and the total volume sampled by the survey is more than 25 million cubic light-years.

The astronomers compared their result with that of the 2dFGRS survey that probed the local Universe, i.e. measures the distortion at the present time. Within current uncertainties, the measurement of this effect provides an independent indication of the need for an unknown extra energy ingredient in the 'cosmic soup', supporting the simplest form of dark energy, the so-called cosmological constant, introduced originally by Albert Einstein. The large uncertainties do not yet exclude the other scenarios, though.

"We have also shown that by extending our measurements over volumes about ten times larger than the VVDS, this technique should be able to tell us whether cosmic acceleration originates from a dark energy component of exotic origin or requires a modification of the laws of gravity," explains Guzzo.

Reference
"A test of the nature of cosmic acceleration using galaxy redshift distortions",
L. Guzzo, M. Pierleoni, B. Meneux, E. Branchini, O. Le Fèvre, C. Marinoni, B. Garilli, J. Blaizot, G. De Lucia, A. Pollo, H. J. McCracken, D. Bottini, V. Le Brun, D. Maccagni, J. P. Picat, R. Scaramella, M. Scodeggio, L. Tresse, G. Vettolani, A. Zanichelli, C. Adami, S. Arnouts, S. Bardelli, M. Bolzonella, A. Bongiorno, A. Cappi, S. Charlot, P. Ciliegi, T. Contini, O. Cucciati, S. de la Torre, K. Dolag, S. Foucaud, P. Franzetti, I. Gavignaud, O. Ilbert, A. Iovino, F. Lamareille, B. Marano, A. Mazure, P. Memeo, R. Merighi, L. Moscardini, S. Paltani, R. Pellò, E. Perez-Montero, L. Pozzetti, M. Radovich, D. Vergani, G. Zamorani & E. Zucca,
Nature 451, 541-544 (31 January 2008), Abstract Link

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Monday, February 11, 2008

Upcoming Physics Conferences

[To add an upcoming physics conference to this list, please send an email to 2Physics@gmail.com ]

February 20-22: Sources and detection of dark matter and dark energy in the universe (Marina del Rey, California, USA)
February 25-29: Nonequilibrium Phenomena (UC, Santa Barbara)
March 15-22: Moriond Cosmology Rencontre (La Thuile, Italy)
March 18-19: BritGrav 8 (York, UK)
March 24-28: Workshop on classical and quantum information theory (Santa Fe, New Mexico)
March 27-29: Astrophysical Tests of Fundamental Physics (Porto, Portugal)
April 20-25: Loops and legs in quantum field theory (Sondershausen, Germany)
May 7-9: Physics of the Universe (Madrid, Spain)
May 12-16: New paths to quantum gravity (Holbaek Bay, Denmark)
May 18-23: Challenges in particle astrophysics (Blois, France)
May 26-30: 8th intl conference on clifford algebras and their applications in mathematical physics (Campinas, Brazil)
June 2-7: Mathematical aspects of quantum chaos (Montréal, Canada)
June 4-6: Recent Developments in Gravity (Thessaloniki, Greece)
June 6-28: Theory and particle physics: the LHC perspective and beyond (Cargese, France)
June 9-13: Hyperbolic Problems (Maryland)
June 9-13: 16th intl conference on ultrafast phenomena (Stresa, Italy)
June 12-14: Post Newton 2008 (Jena, Germany)
June 13-15: Nature and Ontology (Montreal)
June 15-20: 5th intl conference on new developments in photodetection (Aix-les-Bains, France)
June 16-20: LISA Symposium (Barcelona, Spain)
June 17-25: Intl Fermi School of Physics "measurements of neutrino mass" (Varenna, Italy)
June 23-28: RUSGRAV-13 (Moscow, Russia)
June 27- July 5: Erice Simulation school (Erice, Italy)
June 30- July 4: 6th Euromech nonlinear dynamics conference (St Petersburg, Russia)
June 30-July 4: QG2, Quantum Geometry and Quantum Gravity Conference (Nottingham, UK)
July 7-11: Dark Energy and Dark Matter (Lyon, France)
August 25-29: Geometry and Analysis (Stockholm)
August 25-29: 22nd general conference of the condensed matter division of the European Physical Society (Rome, Italy)
August 26-29: Strong and Electroweak Matter (Amsterdam) Contact: sewm08@science.uva.nl
September 7-12: 100 Years after Minkowski (Bad Honnef, Germany)
September 15-19: Raman scattering in materials science (Warsaw, Poland)

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